DENIS-P J1901391-370017: IS A YOUNG VERY LOW-MASS STAR OR A LOW-MASS BROWN DWARF IN CORONA-AUSTRALIS?
DENIS-P J1901391-370017 has been identified as a low-mass brown dwarf in the Corona-Australis cloud. This paper presents our mass estimate of this brown dwarf. The dereddened spectral energy distribution of the source indicates that DENIS-P J1901391-370017 is a very low-mass star, not a low-mass brown dwarf, as previously reported. We also reconfirm that DENIS-P J1901391-370017 is diskless, as previously mentioned in the literature.
Authors
- N. Phan-Bao (ORCID: https://orcid.org/0000-0002-4481-0094)
Publication Details
- Journal
- Tạp chí Khoa học
- Published
- 2024-09-30
- DOI
- https://doi.org/10.54607/hcmue.js.21.9.4459(2024)
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.00